Solar System Formation
Planets & Stars
Orbits & Space Science
Layers of Earth
Earthquakes & Seismic Waves
Earth's Heat & Movement
100

What was the solar system formed from?

A rotating cloud of gas and dust called the solar nebula.

100

What are the two main categories of planets in our solar system?

Terrestrial and Jovian planets.

100

According to Kepler's First Law, what shape are planetary orbits?

Ellipses, with the Sun at one focus.

100

What is the rigid outer mechanical layer of Earth called?

lithosphere

100

What do scientists study to learn about Earth's deep interior?

Seismic waves from earthquakes.

100

Name one major source of heat inside Earth.

Leftover heat from early impacts or heat from radioactive decay.

200

What process allowed small pieces of material to combine into larger bodies and eventually planets?

Accretion

200

Where are dense, rocky planets most likely to form?

Near the central star.

200

When does a planet move fastest in its orbit?

When it is closest to the Sun.

200

Which mechanical layer includes Earth's crust?

lithosphere

200

Which type of seismic wave cannot travel through liquids?

S waves.

200

What process transfers heat through the mantle?

What process transfers heat through the mantle?

Answer: Convection.

300

What event may have triggered the collapse of the original solar nebula?

A nearby supernova.

300

What factor has the greatest influence on how long a star lives?

Its mass.

300

What two measurements are related by Kepler's Third Law?

Orbital period and average distance from the Sun.

300

Which layer is softer and more easily deformed: the lithosphere or asthenosphere?

asthenosphere

300

How do the coils of a stretched spring move when a P wave passes through?

They compress and spread out parallel to the wave’s travel direction.

300

Does mantle convection involve the movement of solid rock or liquid water?

Very slow movement and deformation of solid rock.

400

What began in the central protostar when it became hot and dense enough?

Nuclear fusion

400

Where did many of the heavy elements found on Earth originate?

Supernova explosions.

400

A planet has a semimajor axis of 4 AU. Using P² = a³, what is its orbital period?

8 years. P² = 4³ = 64, so P = 8 years.

400

What three properties generally increase with depth inside Earth?

Temperature, pressure, and density.

400

How do the coils move when an S wave passes through a stretched spring?

Sideways, perpendicular to the wave’s travel direction.

400

How is mantle convection related to Earth's surface?

It is associated with the movement of tectonic plates.

500

Put these stages in order: stellar wind clears gas, planetesimals accrete, nebula collapses, nuclear fusion begins.

Nebula collapses → nuclear fusion begins → planetesimals accrete → stellar wind clears leftover gas.

500

Why are the inner planets mostly rocky while the outer planets are largely gaseous?

The inner nebula was hotter, favoring rocky materials; cooler outer regions allowed gas- and ice-rich planets to develop.

500

What technique uses light to identify the composition of stars and planets?

Spectroscopy; astronomers analyze the light and its spectral features.

500

Where are Earth's tectonic plates located?

In the rigid lithosphere, extending from the surface to approximately 100 km deep in the textbook model.

500

How can scientists locate an earthquake's epicenter?

By comparing P- and S-wave arrival times at at least three seismic stations.

500

Explain the two sources of Earth's internal heat and how that heat relates to tectonic plate movement.

Early impact heat and radioactive decay supply internal heat. Slow mantle convection transfers heat and is associated with tectonic plate motion.